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The Evolutionary Map of the Universe Pilot Survey

  • Ray P. Norris
  • , Joshua Marvil
  • , J. D. Collier
  • , Anna D. Kapinska
  • , Andrew N. O'Brien
  • , L. Rudnick
  • , Heinz Andernach
  • , Jacobo Asorey
  • , Michael J. I. Brown
  • , Marcus Bruggen
  • , Evan Crawford
  • , Jayanne English
  • , Syed Faisal ur Rahman
  • , Miroslav D. Filipovic
  • , Yjan Gordon
  • , Gulay Gurkan
  • , Catherine Hale
  • , Andrew M. Hopkins
  • , Minh T. Huynh
  • , Kim HyeongHan
  • M. James Jee, Baerbel S. Koribalski, Emil Lenc, Kieran Luken, David Parkinson, Isabella Prandoni, Wasim Raja, Thomas H. Reiprich, Christopher J. Riseley, Stanislav S. Shabala, Jaimie R. Sheil, Tessa Vernstrom, Matthew T. Whiting, James R. Allison, C. S. Anderson, Lewis Ball, Martin Bell, John Bunton, T. J. Galvin, Neeraj Gupta, Aidan Hotan, Colin Jacka, Peter J. Macgregor, Elizabeth K. Mahony, Umberto Maio, Vanessa Moss, M. Pandey-Pommier, Maxim A. Voronkov

Research output: Contribution to journalArticlepeer-review

Abstract

We present the data and initial results from the first pilot survey of the Evolutionary Map of the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The survey covers of an area covered by the Dark Energy Survey, reaching a depth of 25–30 rms at a spatial resolution of 11–18 arcsec, resulting in a catalogue of 220 000 sources, of which 180 000 are single-component sources. Here we present the catalogue of single-component sources, together with (where available) optical and infrared cross-identifications, classifications, and redshifts. This survey explores a new region of parameter space compared to previous surveys. Specifically, the EMU Pilot Survey has a high density of sources, and also a high sensitivity to low surface brightness emission. These properties result in the detection of types of sources that were rarely seen in or absent from previous surveys. We present some of these new results here.
Original languageEnglish
Article numbere046
Pages (from-to)1-26
Number of pages26
JournalPublications of the Astronomical Society of Australia
Volume38
DOIs
Publication statusPublished - 7 Sept 2021

Keywords / Materials (for Non-textual outputs)

  • astro-ph.CO
  • astro-ph.IM

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